1996
DOI: 10.1180/minmag.1996.060.401.03
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Distribution of boron, lithium and beryllium in ocean island basalts from French Polynesia: implications for the B/Be and Li/Be ratios as tracers of subducted components

Abstract: The study focuses on the distribution of B, Be, Li, rare earth elements (REE), high-field-strength elements (HFSE), Th, U and Pb in fresh and hydrothermally altered ocean island basalts (OIB) from French Polynesia, and evaluates B/Be and Li/Be ratios as potential tracers of subducted components in the mantle. Hydrothermal solutions affecting the rocks during cooling were derived from meteoric water, sea water and magmatic fluids. The concentrations of REE, HFSE, Th and Be in the OIB were not affected by second… Show more

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Cited by 19 publications
(13 citation statements)
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“…Such a calculated melt in equilibrium with the completely homogenized Group II xenolith Ke 1958/20 would have 4.9 μ g/g Li, 3.2 μ g/g Be and 5.8 μ g/g B (using the average Li, Be and B of ol‐I, opx‐I, and cpx‐I, bulk partition coefficients based on mineral/melt D values of Brenan et al [1998a] and relative modal abundances as given in Table 1; spinel was neglected due to low modal abundances). These values compare well with typical light element budgets of OIB type intraplate basaltic rocks [e.g., Ryan and Langmuir , 1987; Dostal et al , 1996; Ryan et al , 1996; Ryan and Kyle , 2004; Tanaka and Nakamura , 2005; Gméling et al , 2007]. This also holds true for Ce/B and B/Be of the hypothetical melt (Figure 9b), but not for the Li/Yb ratio, which is significantly lower (∼0.5) than in any typical mantle‐derived melt (Figure 9a).…”
Section: Comparison Between Light Elements and Rees: Implications Forsupporting
confidence: 83%
“…Such a calculated melt in equilibrium with the completely homogenized Group II xenolith Ke 1958/20 would have 4.9 μ g/g Li, 3.2 μ g/g Be and 5.8 μ g/g B (using the average Li, Be and B of ol‐I, opx‐I, and cpx‐I, bulk partition coefficients based on mineral/melt D values of Brenan et al [1998a] and relative modal abundances as given in Table 1; spinel was neglected due to low modal abundances). These values compare well with typical light element budgets of OIB type intraplate basaltic rocks [e.g., Ryan and Langmuir , 1987; Dostal et al , 1996; Ryan et al , 1996; Ryan and Kyle , 2004; Tanaka and Nakamura , 2005; Gméling et al , 2007]. This also holds true for Ce/B and B/Be of the hypothetical melt (Figure 9b), but not for the Li/Yb ratio, which is significantly lower (∼0.5) than in any typical mantle‐derived melt (Figure 9a).…”
Section: Comparison Between Light Elements and Rees: Implications Forsupporting
confidence: 83%
“…For consistency, samples were selected from suites analysed mainly at the Centre Geologique et Geophysique, Universite de Montpellier II and St Mary's University, Halifax (Dostal et al 1983(Dostal et al , 1995(Dostal et al , 1998Liotard et al 1986;Dupuy et al 1987Dupuy et al , 1988Dupuy et al , 1989Dupuy et al , 1992Dupuy et al , 1993. As a result, chemical differences between samples are likely to reflect differences in composition as opposed to being artifacts of different analytical methods.…”
Section: Data Preparationmentioning
confidence: 99%
“…Be, B, Li, As, and Sb systematics of high-P, low-T mafic rocks of the Pouébo Terrane. Data for the MORB and OIB fields is from Ludden and Thompson (1979), Chan et al (1992), Dostal et al (1996), Leeman (1996), Leeman and Sisson (1996), Noll et al (1996), Teagle et al (1996), Kamenetsky et al (2000), Neal et al (2002) and Ryan (2002). alent rocks is required to qualitatively evaluate element mobility during subduction.…”
Section: Comparison With Equivalent Protolith Rocksmentioning
confidence: 99%